Add to ORKGThe measurement of non-zero polarization can be used to infer the presence of departures from spherical symmetry in supernovae (SNe). The origin of the majority of the intrinsic polarization observed in SNe is in electron scattering, which induces a wavelength-independent continuum polarization that is generally observed to be low (<1%) for all SN types. The key indicator of asymmetry in SNe is the polarization observed across spectral lines, in particular the characteristic ``inverse P Cygni'' profile. The results of a suite of 900 Monte Carlo radiative transfer simulations are presented here. These simulations cover a range of possible axisymmetric structures (including unipolar, bipolar and equatorial enhancements) for the line forming r...
We study the multi-dimensional geometry of supernova (SN) explosions by means of spectropolarimetric...
We present modeling of line polarization to study the multidimensional geometry of stripped-envelope...
Supernovae of type IIn possess spectral signatures that indicate an intense interaction between the ...
We present the first spectropolarimetric observations of a hydrogen-free superluminous supernova (SL...
Defining the progenitor system and explaining how the explosion proceeds through the star are two diffi...
The explosion processes of supernovae (SNe) are imprinted in their explosion geometries. Here, we st...
The origin of the luminosity of superluminous supernovae (SLSNe) is an unresolved mystery, and a num...
International audienceWe present synthetic single-line and continuum linear-polarization signatures ...
We present a compilation of the geometry measures acquired using optical and IR spectroscopy and opt...
International audienceWe present VLT–FORS spectropolarimetric observations of the type II supernova ...
We present six epochs of optical spectropolarimetry of the Type II supernova (SN) 2023ixf ranging fr...
We present a sequence of eight spectropolarimetric observations monitoring the geometric evolution o...
We briefly review the young field of spectropolarimetry of core-collapse supernovae (SNe). Spectropo...
Detailed spectropolarimetric studies may hold the key to probing the explosion mechanisms and the pr...
We present a compilation of the geometry measures acquired using optical and IR spectroscopy and opt...
We study the multi-dimensional geometry of supernova (SN) explosions by means of spectropolarimetric...
We present modeling of line polarization to study the multidimensional geometry of stripped-envelope...
Supernovae of type IIn possess spectral signatures that indicate an intense interaction between the ...
We present the first spectropolarimetric observations of a hydrogen-free superluminous supernova (SL...
Defining the progenitor system and explaining how the explosion proceeds through the star are two diffi...
The explosion processes of supernovae (SNe) are imprinted in their explosion geometries. Here, we st...
The origin of the luminosity of superluminous supernovae (SLSNe) is an unresolved mystery, and a num...
International audienceWe present synthetic single-line and continuum linear-polarization signatures ...
We present a compilation of the geometry measures acquired using optical and IR spectroscopy and opt...
International audienceWe present VLT–FORS spectropolarimetric observations of the type II supernova ...
We present six epochs of optical spectropolarimetry of the Type II supernova (SN) 2023ixf ranging fr...
We present a sequence of eight spectropolarimetric observations monitoring the geometric evolution o...
We briefly review the young field of spectropolarimetry of core-collapse supernovae (SNe). Spectropo...
Detailed spectropolarimetric studies may hold the key to probing the explosion mechanisms and the pr...
We present a compilation of the geometry measures acquired using optical and IR spectroscopy and opt...
We study the multi-dimensional geometry of supernova (SN) explosions by means of spectropolarimetric...
We present modeling of line polarization to study the multidimensional geometry of stripped-envelope...
Supernovae of type IIn possess spectral signatures that indicate an intense interaction between the ...